<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE dataset SYSTEM "http://tarantella.gsfc.nasa.gov/xml/dataset_048.dtd">
<dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
	<title>A list of stars classified as Supergiants</title>
	<altname type="ADC">5017A</altname>
		<altname type="CDS">V/17A</altname>
		<altname type="brief">A list of Supergiant Stars</altname>
	<reference>
		<source>
<journal>
	<title>A list of stars classified as Supergiants</title>
	<author>
			<initial>D</initial>
			<lastName>Egret</lastName></author>
	<name>Bull. Inform. CDS</name>
	<volume>18</volume>
	<pageno>82</pageno>
		<date>
			<year>1980</year></date>
	<bibcode>1980BICDS..18...82E</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Stars_supergiant.html">Stars, supergiant</keyword></keywords>
	<descriptions>
				<description>
				<para>
    This catalogue is a compilation of about 5000 stars classified as
    supergiants (class I or II) in the literature. The following
    information is given: DM and HD identifications, coordinates,
    photometry, radial velocity and MK classification</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="catalog">
	<title>The list of Supergiants</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>CSI</name>
			<definition>designation
	<footnote footnoteId="???"><para>number=1</para>
			<para>The CSI designation (see Ochsenbein et al. 1980) is made of 3 parts:
    the zone, the number, and a code.
    For a positive number, the code indicates which Durchmusterung the
    zone and number refer to:
    - BD (Bonner  Durchmusterung) for  0 &lt;= code &lt;= 19
    - CD (Cordoba Durchmusterung) for 20 &lt;= code &lt;= 39
    - CPD (Cape Durchmusterung)   for 40 &lt;= code &lt;= 59
    A negative number (constructed from 1950 right ascension) is assigned
    for non-DM stars.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>HD</name>
			<definition>Henry Draper Catalogue Designation</definition>
			<units>---</units></field>
		<field>
			<name>m_HD</name>
			<definition>Multiplicity index on HD number;
                                    a '/' indicates a group of 2 HD numbers</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right Ascension 1950 (hours)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right Ascension 1950 (minutes)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right Ascension 1950 (seconds)</definition>
			<units>s</units></field>
		<field>
			<name>u_RAs</name>
			<definition>for poor position (accuracy 1arcmin)</definition>
			<units>---</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination 1950 (sign)</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination 1950 (degrees)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination 1950 (minutes)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination 1950 (seconds)</definition>
			<units>arcsec</units></field>
		<field>
			<name>GLON</name>
			<definition>Galactic longitude</definition>
			<units>deg</units></field>
		<field>
			<name>GLAT</name>
			<definition>Galactic latitude</definition>
			<units>deg</units></field>
		<field>
			<name>n_Vmag</name>
			<definition>Variability or Duplicity indicator</definition>
			<units>---</units></field>
		<field>
			<name>Vmag</name>
			<definition>Visual magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>u_Vmag</name>
			<definition>Uncertainty flag (:) on Vmag</definition>
			<units>---</units></field>
		<field>
			<name>q_Vmag</name>
			<definition>Quality indicator on Vmag
	<footnote footnoteId="???"><para>number=2</para>
			<para>the quality number (1=poor, 4=good) comes from the UBV catalogue
    by Nicolet (1978);</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>B-V</name>
			<definition>Colour</definition>
			<units>mag</units></field>
		<field>
			<name>q_B-V</name>
			<definition>Quality indicator on B-V
	<footnote footnoteId="???"><para>number=2</para>
			<para>the quality number (1=poor, 4=good) comes from the UBV catalogue
    by Nicolet (1978);</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>U-B</name>
			<definition>Colour</definition>
			<units>mag</units></field>
		<field>
			<name>q_U-B</name>
			<definition>Quality indicator on U-B
	<footnote footnoteId="???"><para>number=2</para>
			<para>the quality number (1=poor, 4=good) comes from the UBV catalogue
    by Nicolet (1978);</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Gflag</name>
			<definition>'G' when Geneva photometry exists</definition>
			<units>---</units></field>
		<field>
			<name>Uflag</name>
			<definition>'U' when uvby photometry exists</definition>
			<units>---</units></field>
		<field>
			<name>RVel</name>
			<definition>Radial Velocity from Wilson (1953)
                                    or Evans (1967)</definition>
			<units>km/s</units></field>
		<field>
			<name>q_RVel</name>
			<definition>Quality on Radial Velocity
                                    (A=good, E=very poor)</definition>
			<units>---</units></field>
		<field>
			<name>n_Sp</name>
			<definition>Dispersive system used, or quality
                                    from Houk's catalogue (when Sep='X')
	<footnote footnoteId="???"><para>number=3</para>
			<para>The MK classification from N. Houk (1975, 1978) includes a quality
    from 1 (good) to 4 (poor), a '+' for spectra classified in other sources,
    and 'X' when several spectra were available. When Sep is a '/', the
    classification is from Jaschek (1978)
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Sep</name>
			<definition>Separator ('X' when Sp is from Houk)</definition>
			<units>---</units></field>
		<field>
			<name>Sp</name>
			<definition>Spectral classification
	<footnote footnoteId="???"><para>number=3</para>
			<para>The MK classification from N. Houk (1975, 1978) includes a quality
    from 1 (good) to 4 (poor), a '+' for spectra classified in other sources,
    and 'X' when several spectra were available. When Sep is a '/', the
    classification is from Jaschek (1978)
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Francois Ochsenbein</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1995</year><month>Jul</month><day>12</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>  * June 1980: catalogue prepared and archived at CDS
  * 12-Jul-1995: the catalogue was reformatted at CDS:
    => elimination of record headers "5017A1"
    => creation of a dedicated column for the ':' uncertainty flag u_Vmag
       which was previously embedded in the Vmag column
    => addition of the standard documentation</para></revision></revisions></history>
	<identifier>V_17A.xml</identifier></dataset>
